How can you determine the diameter of the sun?

1 Answer
Feb 23, 2016

If \theta is the angular diameter of the sun as measured from earth and D is the distance to the sun, then the diameter of the sun d_{sun} is
d_{sun}=2*D*tan (\theta/2) .
Using the small angle approximation (tan\theta~=\theta in radians)
d_{sun}= D*\theta in \theta radians or
d_{sun}= D*\pi/180*\theta in \theta degrees.

Explanation:

Draw the sun, given the sun some size, draw a point to represent the location of the earth (this does NOT need to be to scale).
Draw a line from the location of the earth to the center of the sun.
Draw the diameter of the sun at right angles to this like.
Make an isosceles triangle by connecting the ends of the diameter to the loctaion of the earth. Should look something like this. enter image source here

\theta the angular size of the sun is the angle bound by the diameter.

\theta/2 is the little angle in the two right angle triangles.

tan(\theta/2)=r_{sun}/D

rearranging we have

r_{sun}=D tan(\theta/2).

since d_{sun}=2* r_{sun}

d_{sun}=2*D *tan(\theta/2).
Using the small angle approximation (which only works in radians) we have,
d_{sun}=2*D* \theta/2=D *\theta_{radians} .
If we have \theta in degrees we can convert using \theta_{radians}=pi/180 \theta_{degrees}
giving
d_{sun}=pi/180 D *\theta_{degrees}

note that \theta_{degrees} is around half a degree.